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    UCLA Dark Matter 2025

    Mar 24 – 27, 2025
    UCLA Physics and Astronomy Building 1-425
    US/Pacific timezone

    darkmatter@physics.ucla.edu

    Session

    SESSION 4: Direct Dark Matter Detection (CHAIR: Alvine Kamaha -UCLA)

    Mar 24, 2025, 3:50 PM
    UCLA Physics and Astronomy Building 1-425

    UCLA Physics and Astronomy Building 1-425

    475 Portola Plaza, Los Angeles, CA 90095 darkmatter@physics.ucla.edu

    Presentation materials

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    1. 193. Direct Detection with Xenon
      Elena Aprile
      3/24/25, 3:50 PM
      Talk

      NA

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    2. 194. Direct Detection with Argon
      Cristiano Galbiati
      3/24/25, 4:15 PM
      Talk

      NA

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    3. 195. Direct Detection with Cryogenic Solid State Detectors
      Sunil Golwala
      3/24/25, 4:40 PM
      Talk

      NA

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    4. 196. The Status of Sub-GeV Direct Detection
      Rouven Essig
      3/24/25, 5:05 PM
      Talk

      NA

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    5. 6. PaleoDetectors (Ancient Minerals from Deep Underground)
      Prof. Katherine Freese (University of Texas)
      3/24/25, 5:30 PM
      Talk

      Paleo-detectors are a proposed experimental technique to search for dark matter (DM). In lieu of the conventional approach of operating a tonne-scale real-time detector to search for DM-induced nuclear recoils, paleo-detectors take advantage of small samples of naturally occurring rocks on Earth that have been deep underground (≳5 km), accumulating nuclear damage tracks from recoiling nuclei...

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